A-type main-sequence star and Gamma Trianguli

Shortcuts: Differences, Similarities, Jaccard Similarity Coefficient, References.

Difference between A-type main-sequence star and Gamma Trianguli

A-type main-sequence star vs. Gamma Trianguli

An A-type main-sequence star (A V) or A dwarf star is a main-sequence (hydrogen-burning) star of spectral type A and luminosity class V. These stars have spectra which are defined by strong hydrogen Balmer absorption lines. Gamma Trianguli (Gamma Tri, γ Trianguli, γ Tri) is a star in the constellation Triangulum located approximately 112 light years from Earth.

Similarities between A-type main-sequence star and Gamma Trianguli

A-type main-sequence star and Gamma Trianguli have 5 things in common (in Unionpedia): Altair, Debris disk, Effective temperature, Star, Stellar classification.

Altair

Altair, also designated Alpha Aquilae (α Aquilae, abbreviated Alpha Aql, α Aql), is the brightest star in the constellation of Aquila and the twelfth brightest star in the night sky.

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Debris disk

A debris disk is a circumstellar disk of dust and debris in orbit around a star.

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Effective temperature

The effective temperature of a body such as a star or planet is the temperature of a black body that would emit the same total amount of electromagnetic radiation.

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Star

A star is type of astronomical object consisting of a luminous spheroid of plasma held together by its own gravity.

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Stellar classification

In astronomy, stellar classification is the classification of stars based on their spectral characteristics.

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The list above answers the following questions

What A-type main-sequence star and Gamma Trianguli have in common
What are the similarities between A-type main-sequence star and Gamma Trianguli

A-type main-sequence star and Gamma Trianguli Comparison

A-type main-sequence star has 38 relations, while Gamma Trianguli has 36. As they have in common 5, the Jaccard index is 6.76% = 5 / (38 + 36).

References

This article shows the relationship between A-type main-sequence star and Gamma Trianguli. To access each article from which the information was extracted, please visit:

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